The main-sequence of the star.

Question

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Answer 1

Question

Chapter 12, Problem 1RQ

To determine

The main-sequence of the star.

Expert Solution & Answer

Answer to Problem 1RQ

A main sequence star is generated energy by fusion of hydrogen into helium in its core.

Explanation of Solution

In the H-R diagram, a star is located on the main-sequence. Get causally brighter with age.

That should be in Hydrostatic Equilibrium.
That should be in Thermal Equilibrium.
That should generate the energy by fusion of hydrogen into helium in its core.
These conditions are necessary, if not followed the star must left the main-sequence.

Gravity pulls each and every atom in a star towards the center, but its weight is balanced by the outward pressure of the hot gas which is inside the star. In that star, gases are heated by the nuclear reactions. The energy travels toward outside and its support the weight pressing down on it. At the beginning of the fusion, deuterium is burning.

Conclusion:

Therefore, a main sequence star is generated energy by fusion of hydrogen into helium in its core.

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Students have asked these similar questions

What evidence is there that star formation has occurred recently?

The place on the H–R diagram where contracting protostars first become visible is a. the horizontal branch. b. the instability strip. c. the birth line. d. the zero-age main sequence. e. none of the above.

Describe the forces acting on a star during the main sequence period of its life?

Answer 2

Question

Chapter 12, Problem 1RQ

To determine

The main-sequence of the star.

Expert Solution & Answer

Answer to Problem 1RQ

A main sequence star is generated energy by fusion of hydrogen into helium in its core.

Explanation of Solution

In the H-R diagram, a star is located on the main-sequence. Get causally brighter with age.

That should be in Hydrostatic Equilibrium.
That should be in Thermal Equilibrium.
That should generate the energy by fusion of hydrogen into helium in its core.
These conditions are necessary, if not followed the star must left the main-sequence.

Gravity pulls each and every atom in a star towards the center, but its weight is balanced by the outward pressure of the hot gas which is inside the star. In that star, gases are heated by the nuclear reactions. The energy travels toward outside and its support the weight pressing down on it. At the beginning of the fusion, deuterium is burning.

Conclusion:

Therefore, a main sequence star is generated energy by fusion of hydrogen into helium in its core.

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Answer 3

Question

Chapter 12, Problem 1RQ

To determine

The main-sequence of the star.

Expert Solution & Answer

Answer to Problem 1RQ

A main sequence star is generated energy by fusion of hydrogen into helium in its core.

Explanation of Solution

In the H-R diagram, a star is located on the main-sequence. Get causally brighter with age.

That should be in Hydrostatic Equilibrium.
That should be in Thermal Equilibrium.
That should generate the energy by fusion of hydrogen into helium in its core.
These conditions are necessary, if not followed the star must left the main-sequence.

Gravity pulls each and every atom in a star towards the center, but its weight is balanced by the outward pressure of the hot gas which is inside the star. In that star, gases are heated by the nuclear reactions. The energy travels toward outside and its support the weight pressing down on it. At the beginning of the fusion, deuterium is burning.

Conclusion:

Therefore, a main sequence star is generated energy by fusion of hydrogen into helium in its core.

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Subscribe now to access step-by-step solutions to millions of textbook problems written by subject matter experts!

Answer 4

Question

Chapter 12, Problem 1RQ

To determine

The main-sequence of the star.

Expert Solution & Answer

Answer to Problem 1RQ

A main sequence star is generated energy by fusion of hydrogen into helium in its core.

Explanation of Solution

In the H-R diagram, a star is located on the main-sequence. Get causally brighter with age.

That should be in Hydrostatic Equilibrium.
That should be in Thermal Equilibrium.
That should generate the energy by fusion of hydrogen into helium in its core.
These conditions are necessary, if not followed the star must left the main-sequence.

Gravity pulls each and every atom in a star towards the center, but its weight is balanced by the outward pressure of the hot gas which is inside the star. In that star, gases are heated by the nuclear reactions. The energy travels toward outside and its support the weight pressing down on it. At the beginning of the fusion, deuterium is burning.

Conclusion:

Therefore, a main sequence star is generated energy by fusion of hydrogen into helium in its core.

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Subscribe now to access step-by-step solutions to millions of textbook problems written by subject matter experts!

Answer 5

Chapter 12, Problem 1RQ

To determine

The main-sequence of the star.

Expert Solution & Answer

Answer to Problem 1RQ

A main sequence star is generated energy by fusion of hydrogen into helium in its core.

Explanation of Solution

In the H-R diagram, a star is located on the main-sequence. Get causally brighter with age.

That should be in Hydrostatic Equilibrium.
That should be in Thermal Equilibrium.
That should generate the energy by fusion of hydrogen into helium in its core.
These conditions are necessary, if not followed the star must left the main-sequence.

Gravity pulls each and every atom in a star towards the center, but its weight is balanced by the outward pressure of the hot gas which is inside the star. In that star, gases are heated by the nuclear reactions. The energy travels toward outside and its support the weight pressing down on it. At the beginning of the fusion, deuterium is burning.

Conclusion:

Therefore, a main sequence star is generated energy by fusion of hydrogen into helium in its core.

Answer 6

Chapter 12, Problem 1RQ

To determine

The main-sequence of the star.

Expert Solution & Answer

Answer to Problem 1RQ

A main sequence star is generated energy by fusion of hydrogen into helium in its core.

Explanation of Solution

In the H-R diagram, a star is located on the main-sequence. Get causally brighter with age.

That should be in Hydrostatic Equilibrium.
That should be in Thermal Equilibrium.
That should generate the energy by fusion of hydrogen into helium in its core.
These conditions are necessary, if not followed the star must left the main-sequence.

Gravity pulls each and every atom in a star towards the center, but its weight is balanced by the outward pressure of the hot gas which is inside the star. In that star, gases are heated by the nuclear reactions. The energy travels toward outside and its support the weight pressing down on it. At the beginning of the fusion, deuterium is burning.

Conclusion:

Therefore, a main sequence star is generated energy by fusion of hydrogen into helium in its core.

Answer 7

Chapter 12, Problem 1RQ

To determine

The main-sequence of the star.

Answer 8

Expert Solution & Answer

Answer to Problem 1RQ

A main sequence star is generated energy by fusion of hydrogen into helium in its core.

Answer 9

Expert Solution & Answer

Answer 10

Expert Solution & Answer

Answer 11

Explanation of Solution

In the H-R diagram, a star is located on the main-sequence. Get causally brighter with age.

That should be in Hydrostatic Equilibrium.
That should be in Thermal Equilibrium.
That should generate the energy by fusion of hydrogen into helium in its core.
These conditions are necessary, if not followed the star must left the main-sequence.

Gravity pulls each and every atom in a star towards the center, but its weight is balanced by the outward pressure of the hot gas which is inside the star. In that star, gases are heated by the nuclear reactions. The energy travels toward outside and its support the weight pressing down on it. At the beginning of the fusion, deuterium is burning.

Conclusion:

Therefore, a main sequence star is generated energy by fusion of hydrogen into helium in its core.

Answer 12

Ch. 12 - Prob. 1RQ Ch. 12 - Prob. 2RQ Ch. 12 - Prob. 3RQ Ch. 12 - Prob. 4RQ Ch. 12 - Prob. 5RQ Ch. 12 - Describe the law of hydrostatic equilibrium.Ch. 12 - Prob. 7RQ Ch. 12 - Prob. 8RQ Ch. 12 - Prob. 9RQ Ch. 12 - Prob. 10RQ

The main-sequence of the star.

Concept explainers

The main-sequence of the star.

Answer to Problem 1RQ

Explanation of Solution

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Chapter 12 Solutions